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Black Hole Thermodynamics and Geometry

  • Stefano Bellucci
  • Alessio Marrani
  • Sergio Ferrara
Part of the Lecture Notes in Physics book series (LNP, volume 701)

Abstract

In the previous section we have seen that, in the context of nV -fold, N = 2, d = 4 MESGT, the fundamental properties of 4-d extreme BHs may be described by the “BH effective potential” function V (z, z; p, q), and in particular by its critical points in the moduli space M z , z , which is endowed with a (regular) special Kähler geometry. New insights can be gained by considering the formalism of the geometric approach to the thermodynamical fluctuation theory. Once again, we will mainly follow Ferrara, Gibbons, and Kallosh [55] (for a complete review, see, e.g., [82]).

Keywords

Modulus Space Black Hole Thermodynamic Intensive Variable Schwarz Lemma Extensive Charge 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer 2006

Authors and Affiliations

  • Stefano Bellucci
    • 1
  • Alessio Marrani
    • 2
  • Sergio Ferrara
    • 3
  1. 1.Istituto Nazionale di Fisica NucleareFrascati (Rome)Italy
  2. 2.Istituto Nazionale di Fisica NucleareFrascati (Rome)Italy
  3. 3.Physics DepartmentCERNSwitzerland

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